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eso-midas-doc-13SEPpl1.2-3.mga5.i586.rpm

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<H1><A NAME="SECTION001820000000000000000">
Installation</A>
</H1>
The <B>98NOV</B> release of ESO-MIDAS can run on most UNIX systems, and
is most likely to run under DEC/VMS 4.7 and DEC/OPEN-VMS 6.0 (or higher). 
If you are going to install ESO-MIDAS on your system you have
retrieved a copy of this release through ftp. However, as have been 
announced, as of 1995 new applications are not tested automatically on
VMS/Open VMS systems.

<P>
The monitor and low level interfaces are coded in C which means the 
portable MIDAS requires a C compiler for installation. Many 
applications are written in FORTRAN-77 and can therefore only be 
installed if either a FORTRAN-77 compiler or a FORTRAN-to-C 
convertion package (<I>e.g.</I> <TT>f2c</TT> for UNIX) is 
available. The installation of MIDAS has been certified with the
public domain GNU ANSI-C compiler which can be obtained from the 
Free Software Foundation, and verified with the quality control tool 
Purify from Pure-Software. 

<P>
The instructions for installation are given in separate documents for
either VMS or UNIX systems which are included in the distribution kit.
Read the appropriate one carefully and proceed as described (the
procedure may have been modified compared with previous
installations!). Basic knowledge of your local operating system (e.g.
VMS or UNIX) is assumed and required.

<P>
One area may require special attention during the first installation.
It relates to the image display interfaces that, for MIDAS, must
conform to the standard IDI interfaces. IDI's are provided only for 
the X-Window system, Version 11. For other display devices a
set of IDI routines has to be written.

<P>
For a few commands the NAG mathematical library is required.  If you
do not have this library MIDAS can still be installed, however, some
commands may not be available.  In future versions we will try to
reduce our dependency on NAG.  A list of programs using NAG and the
routines are given in Section&nbsp;<A HREF="node215.html#nag-dep">D.5</A>.

<P>
Starting with the 89NOV release a separate installation of the lower
level AGL library is no longer required. The library, i.e. those parts
needed for the MIDAS plot facilities, is fully integrated within the
MIDAS directory structure and will be generated as every other MIDAS
subroutine library. For a full installation of the AGL library refer
to the Astronet Documentation Facility, Trieste.

<P>
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<ADDRESS>
<I>Petra Nass</I>
<BR><I>1999-06-09</I>
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